A composite image of the close environment of Beta Pictoris as seen in near infrared light. The outer part of the image shows the reflected light on the dust disc, as observed with the ADONIS instrument on ESO's 3.6 m telescope; the inner part is the innermost part of the system, as seen at 3.6 microns with NACO on the Very Large Telescope. Beta Pictoris b is more than 1000 times fainter than its host star. Image Credit/Caption: ESO/A.-M. Lagrange et al